So, this paper is organized as follows: Section 2 is briefly devoted
to charged squashed Kaluza-Klein Gödel black hole background. In
section 3 we use the Bozza's method [1]}, [2]} to obtain
the deflection angle and other parameters of strong gravitational
lensing as well as variation of them with extra dimension,
Gödel parameter and charge of black hole . In section 4, we
suppose that the supermassive object at the center of our galaxy can
be considered by the metric of charged squashed Kaluza-Klein
Gödel black hole. Then, we evaluate the numerical results for
the coefficients and observables in the strong gravitational lensing
. In the last Section, we present a summary of our work.
